Mount Cuba
Astronomical Observatory
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The FT from the first light curve of G29-38 for DAMP17. The data is from Ogloza Waldemar, and was taken on Nov 2. The light curve shows a dominant peak at ~879 s, with numerous additional smaller amplitude peaks.
FT from Nov 5 (UT) from MCAO. The FT shows a complex region of power between 1000 and 2000 microHz. G29-38 is complicated. We need more data:)
FT using data up to Nov 7 (UT) . It includes dta from adyu, mcao, suho, pjmo, and cdk5. The FT shows a complex region of power between 1000 and 2000 microHz. G29-38 is complicated. There are frequencies at 1114.8, 1166,8, 1292.8, 1383.9, 1470.2, 2000.8, 2282.0, 2492.1, and 3522.7 microHz. These frequencies are still under analysis, so this is by no means a final list. Please note the change in x scale from the previous two figures.